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Author manuscript, published in "The 7th European Conference on <strong>Antennas</strong> and Propagation, GOTHENBURG : Sweden (2013)"<br />

<strong>Connected</strong> <strong>Spiral</strong> <strong>Antennas</strong> <strong>for</strong> <strong>Wideband</strong> <strong>Circularly</strong><br />

<strong>Polarized</strong> Antenna Array, Experimental Investigations<br />

Mohammed Serhir 1 , Regis Guivarc’h 2<br />

1 Département de Recherche en Électromagnétisme, Supelec, Gif-sur-Yvette 91192, France (mohammed.serhir@supelec.fr)<br />

2 Laboratory SONDRA, Supelec, 91192 Gif-sur-Yvette, France (regis.guinvarch@supelec.fr).<br />

hal-00834795, version 1 - 17 Jun 2013<br />

Abstract—A cavity backed array of 5 connected spiral<br />

antennas is presented. The circular polarization is generated<br />

using mono polarized spirals in an alternating configuration<br />

RHCP and LHCP. Due to the connection between spirals, the<br />

currents in the arms of one spiral flow into the arms of the<br />

adjacent spirals. The currents transmitted to the opposite<br />

polarized neighboring spiral radiate the same polarization. The<br />

proposed antenna array allows more than 500MHz bandwidth<br />

while being dual polarized and steerable +/- 30deg. The<br />

per<strong>for</strong>mance of the constructed array is presented and validated<br />

using electromagnetic simulations and radiation pattern<br />

measurements.<br />

Index Terms— antenna array, circular polarization<br />

I. INTRODUCTION<br />

RADAR applications and synthetic aperture radar mapping<br />

require wideband phased arrays. For these applications, spiral<br />

antenna is an interesting broadband structure since its working<br />

principle is governed by simple rules.<br />

In fact, the spiral antenna bandwidth minimum frequency<br />

(VSWR


hal-00834795, version 1 - 17 Jun 2013<br />

Figure 2. The elementary spiral antenna (left) and its feeding system (right)<br />

Figure 3. Calculated reflection coefficient of the elementary spiral<br />

The elementary spiral antenna feeding system is made of<br />

two RG-10 coaxial cables soldered together where the inner<br />

conductor of each cable is connected to the spiral arms. Doing<br />

this, the impedance between inner conductors (seen by the<br />

antenna) is also about 100Ω. On the other coaxial cables end a<br />

180° hybrid coupler is used to generate two opposed-phase<br />

signals. This versatile excitation technique can be generalized<br />

to any symmetrical structure <strong>for</strong> which the input impedance is<br />

around 100Ω. Using the electromagnetic simulation software<br />

CST Microwave Studio [4] we calculate the spiral antenna<br />

reflection coefficient as a function of the frequency when it is<br />

excited by the feeding system described above.<br />

As it can be seen from Fig. 3, the antenna S11


and simulated far-field radiation pattern resulting from the<br />

prototype presented in Fig. 7. As it can be seen a good<br />

behavior agreement is noticed. Based on measurement data,<br />

the spiral array has a 650MHz bandwidth from 0.85GHz to<br />

1.5GHz. This bandwidth is confirmed by a good S11 (below-<br />

10dB).<br />

in Fig. 9, the use of the lumped resistive loads does not affect<br />

drastically the radiation pattern.<br />

without resistive loads<br />

Figure 5. Measured S11 coefficients as a function of the frequency<br />

hal-00834795, version 1 - 17 Jun 2013<br />

Figure 6. Comparison of the simulation and measurement Axial Ratio as a<br />

function of the frequency in the broadside direction (θ=0°).<br />

resistive loads<br />

Figure 7. The antenna array with lumped resistive loads.<br />

with resistive loads<br />

without resistive loads<br />

Figure 8. Axial Ratio issued from simulation and measurement data as a<br />

function of the frequency in θ=0° direction <strong>for</strong> spirals with resistive loads.<br />

In Fig. 9, the measured electric field over a hemisphere (-<br />

90°≤θ≤90° and 0≤φ≤180) is presented <strong>for</strong> frequencies inside<br />

the antenna array bandwidth ([0.85GHz 1.35GHz]). As shown,<br />

with resistive loads<br />

Figure 9. Radiation pattern of the spiral array in two different frequencies<br />

0.86GHz and 1.34GHz.


IV.<br />

CONCLUSION<br />

A versatile and efficient cavity backed circularly polarized<br />

array of spiral antenna has been presented. This spiral antenna<br />

array guarantees 500MHz bandwidth where the VSWR is less<br />

than 2 and the axial ration less than 3dB. In this paper we have<br />

excited port2 and port4 to reach the right hand circularly<br />

polarized array (RH). To achieve the left hand circular<br />

polarization (LH) port 1, port 3 and port 5 have to be excited.<br />

Consequently this antenna array structure allows us to realize<br />

LHCP and RHCP polarization. The minimum frequency of the<br />

array is less than the minimum frequency of a single spiral<br />

antenna composing the array structure.<br />

REFERENCES<br />

[1] R. G. Corzine and J. A. Mosko, Four-Arm <strong>Spiral</strong> <strong>Antennas</strong>. Boston,<br />

MA: Artech House, 1990.<br />

[2] R. Guinvarc'h and R.L. Haupt, “Connecting spirals <strong>for</strong> wideband dual<br />

polarization phased array,” <strong>Antennas</strong> and Propagation, IEEE<br />

Transactions on, vol.59, no.12, pp.4534-4541, Dec. 2011<br />

[3] M. McFadden, W. R. Scott Jr.,” Analysis of the Equiangular <strong>Spiral</strong><br />

Antenna on a Dielectric Substrate” <strong>Antennas</strong> and Propagation, IEEE<br />

Transactions on, vol.55, no.11, pp.3163-3171, Nov. 2007<br />

[4] CST Microwave Studio, Tutorial<br />

hal-00834795, version 1 - 17 Jun 2013

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